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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Feldspathic clast populations in polymict ureilites: Stalking the missing basalts from the ureilite parent body
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Feldspathic clast populations in polymict ureilites: Stalking the missing basalts from the ureilite parent body

机译:多微生物尿素岩中的长石性岩屑种群:从尿素岩母体中追踪缺失的玄武岩

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摘要

Polymict ureilites DaG 164/165, DaG 319, DaG 665, and EET 83309 are regolith breccias composed mainly of monomict ureilite-like material, but containing similar to2 vol% of feldspathic components. We characterized 171 feldspathic clasts in these meteorites in terms of texture, mineralogy, and mineral compositions. Based on this characterization we identified three populations of clasts, each of which appears to represent a common igneous (generally basaltic) lithology and whose mafic minerals show a normal igneous fractionation trend of near-constant Fe/Mn ratio over a range of Fe/Mg ratios that extend to much higher values than those in monomict ureilites. The melts represented by these populations are unlikely to be impact melts, because the ubiquitous presence of carbon in polymict ureilites (the regolith of the ureilite parent body) implies that impact melts would have crystallized under conditions of carbon redox control and therefore have highly magnesian mafic mineral compositions with constant Mn/Mg ratio. Therefore, these melts appear to be indigenous products of igneous differentiation on the ureilite parent body (UPB), complementary to the olivine-pigeonite residues represented by the majority of monomict ureilites.The most abundant population is characterized by albitic plagioclase in association with pyroxenes, phosphates, ilmenite, silica, and incompatible-element enriched glass. Model calculations suggest that it formed by extensive fractional crystallization of the earliest melt(s) of precursor materials from which the most magnesian (shallowest) olivine-pigeonite ureilites formed. A less abundant population, characterized by labradoritic plagioclase, may have formed from melts complementary to more ferroan olivine-pigeonite ureilites. and derived from deeper in the UPB. The third population, characterized by the presence of olivine and augite, could only have formed from melts produced at greater depths in the UPB than the olivine-pigeonite ureilites. Many other feldspathic clasts cannot be positively associated with any of these three populations, because their mafic mineral compositions exhibit carbon redox control. However, they may be products of early crystallization of basaltic melts produced on the UPB, before carbon was exhausted by reduction.Partial melting on the ureilite parent body was a fractional (or incremental) process. Melts were produced early in UPB history, and most likely extracted rapidly, thus preserving primitive chemical and oxygen isotopic signatures in the residues. Copyright (C) 2004 Elsevier Ltd.
机译:多微片状绢云母DaG 164/165,DaG 319,DaG 665和EET 83309是重水辉石角砾岩,主要由类单片绢云母状物质组成,但含有约2%(体积)的长石成分。我们从质地,矿物学和矿物组成方面对这些陨石中的171个长石碎屑进行了表征。基于此特征,我们确定了三类碎屑,每一个碎屑似乎代表着一种常见的火成岩(通常是玄武岩)岩性,并且其镁铁质矿物在一定的Fe / Mg范围内显示出接近恒定的Fe / Mn比的正常火成岩分馏趋势。比率扩展到比单分子尿素岩更高的值。这些人群代表的熔体不太可能是冲击熔体,因为在多微晶硅藻土中普遍存在碳(尿素体母体的重晶石)意味着冲击熔体在控制碳氧化还原的条件下会结晶,因此具有高镁质镁铁质镁铁质。 Mn / Mg比恒定的矿物成分。因此,这些熔体似乎是在尿素石母体(UPB)上火成岩分化的本地产物,与大多数单分子尿素石所代表的橄榄石-磷灰石残留物互补。最丰富的种群特征是与辉石相结合的斜生斜长石,磷酸盐,钛铁矿,二氧化硅和不相容元素丰富的玻璃。模型计算表明,它是由前体材料最早的熔体的广泛分级结晶形成的,该熔体形成了镁质(最浅)的橄榄石-辉绿岩点胶石。少量的特征为拉长斜长石的岩浆可能是由与更多的二茂铁橄榄石-辉绿岩胶体互补的熔体形成的。并源自UPB的更深层次。第三特征是橄榄石和钠长石的存在,只能由UPB的深度大于橄榄石-绿皮土点石矿的熔体形成。许多其他长石屑碎屑不能与这三个种群中的任何一个正相关,因为它们的镁铁质矿物成分具有碳氧化还原控制能力。但是,它们可能是UPB上产生的玄武质熔体早期结晶的产物,然后碳被还原消耗掉了。在尿素石母体上的部分熔融是分步(或增量)过程。熔化物是在UPB历史的早期产生的,很可能是迅速提取的,因此在残渣中保留了原始的化学和氧同位素特征。版权所有(C)2004 Elsevier Ltd.

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